Mid-infrared interferometry of massive young stellar objects*

Authors :: Linz, H.
Henning, Th.
Feldt, M.
Pascucci, I.
van Boekel, R.
Men'shchikov, A.
Stecklum, B.
Chesneau, O.
Ratzka, Th.
Quanz, S. P.
Leinert, Ch.
Waters, L. B. F. M.
Zinnecker, H.
Linz, H.
Henning, Th.
Feldt, M.
Pascucci, I.
van Boekel, R.
Men'shchikov, A.
Stecklum, B.
Chesneau, O.
Ratzka, Th.
Quanz, S. P.
Leinert, Ch.
Waters, L. B. F. M.
Zinnecker, H.
Source :: Astronomy and Astrophysics; October 2009, Vol. 505 Issue: 2 p655-661, 7p
Publication Year :: 2009
Abstract: Context. Our knowledge of the inner structure of embedded massive young stellar objects is still quite limited. Thus, it is difficult to decide to what extent the mass accumulation onto forming massive stars differs from the process of low-mass star formation.

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